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News/Events

November 5 2014 -
ADMX Professor Gray Rybka is featured in a conversation with Harry Nelson of LUX-ZEPLIN and Tali Figueroa-Feliciano of SuperCDMS regarding "second-generation" dark matter experiments in a Q&A session moderated by The Kavli Foundation published on space.com.

The Axion Dark Matter
eXperiment (ADMX) uses a
resonant microwave cavity within in a
large superconducting magnet to search for
cold dark matter axions in the
local galactic dark matter
halo. Sited at the
Center for Experimental
Physics and Astrophysics at
the University of Washington,
ADMX is a large collaborative
effort with researchers from
universities and laboratories
around the world. ADMX will soon implement its dilution refrigerator and begin the Gen 2 data schedule.

ADMX will soon be sensitive to even the more weakly coupled
dark matter axions in the range 1μeV to 10μeV.
Target sensitivity for higher frequency R&D is also shown.